J. Pétri
Constraining the magnetic field geometry of the millisecond pulsar PSRJ0030+0451 from joint radio, thermal X-ray, and γ-ray emission
Pétri, J.; Guillot, S.; Guillemot, L.; Cognard, I.; Theureau, G.; Grießmeier, J. M.; Bondonneau, L.; González-Caniulef, D.; Webb, N.; Jankowski, F.; Kravtsov, I. P.; McKee, J. W.; Carozzi, T. D.; Cecconi, B.; Serylak, M.; Zarka, P.
Authors
S. Guillot
L. Guillemot
I. Cognard
G. Theureau
J. M. Grießmeier
L. Bondonneau
D. González-Caniulef
N. Webb
F. Jankowski
I. P. Kravtsov
J. W. McKee
T. D. Carozzi
B. Cecconi
M. Serylak
P. Zarka
Abstract
Context. With the advent of multi-wavelength electromagnetic observations of neutron stars - spanning many decades in photon energies - from radio wavelengths up to X-rays and γ-rays, it has become possible to significantly constrain the geometry and the location of the associated emission regions. Aims. In this work, we use results from the modelling of thermal X-ray observations of PSR J0030+0451 from the Neutron Star Interior Composition Explorer (NICER) mission and phase-aligned radio and γ-ray pulse profiles to constrain the geometry of an off-centred dipole that is able to reproduce the light curves in these respective bands simultaneously. Methods. To this aim, we deduced a configuration with a simple dipole off-centred from the location of the centre of the thermal X-ray hot spots. We show that the geometry is compatible with independent constraints from radio and -ray pulsations only, leading to a fixed magnetic obliquity of α ≈ 75° and a line-of-sight inclination angle of ζ ≈ 54°. Results. We demonstrate that an off-centred dipole cannot be rejected by accounting for the thermal X-ray pulse profiles. Moreover, the crescent shape of one spot is interpreted as the consequence of a small-scale surface dipole on top of the large-scale off-centred dipole.
Citation
Pétri, J., Guillot, S., Guillemot, L., Cognard, I., Theureau, G., Grießmeier, J. M., …Zarka, P. (2023). Constraining the magnetic field geometry of the millisecond pulsar PSRJ0030+0451 from joint radio, thermal X-ray, and γ-ray emission. Astronomy and Astrophysics, 680, Article A93. https://doi.org/10.1051/0004-6361/202346913
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 5, 2023 |
Online Publication Date | Dec 15, 2023 |
Publication Date | Dec 1, 2023 |
Deposit Date | Jan 8, 2024 |
Publicly Available Date | Jan 9, 2024 |
Journal | Astronomy and Astrophysics |
Print ISSN | 0004-6361 |
Electronic ISSN | 1432-0746 |
Publisher | EDP Sciences |
Peer Reviewed | Peer Reviewed |
Volume | 680 |
Article Number | A93 |
DOI | https://doi.org/10.1051/0004-6361/202346913 |
Keywords | stars: neutron; pulsars: individual: PSR J0030+0451; stars: rotation; magnetic fields; gamma rays: stars; X-rays: stars |
Public URL | https://hull-repository.worktribe.com/output/4501029 |
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Copyright Statement
© The Authors 2023
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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